
\begin{table*}[t]
  \centering
  \begin{tabular}{ l c | c c c c c c c c }
    \hline
    \multicolumn{10}{|c|}{Cosmological models with massless neutrinos} \\
    \hline
    \hline
    Acronym & Model & $\Omega_m$ & $\Omega_b$ & $\Omega_\Lambda$ & $h_0$ & $\sigma_8$ & $n_s$ & $w_0$ & $w_a$ \\
    \hline
    CCL1 & flat $\Lambda$CDM & 0.3 & 0.05 & 0.7 & 0.7 & 0.8 & 0.96 & -1 & 0 \\
    CCL2 & $w$CDM & 0.3 & 0.05 & 0.7 & 0.7 & 0.8 & 0.96 & -0.9 & 0  \\
    CCL3 & $w$CDM & 0.3 & 0.05 & 0.7 & 0.7 & 0.8 & 0.96 & -0.9 & 0.1  \\
    CCL4 & open $w$CDM & 0.3 & 0.05 & 0.65 & 0.7 & 0.8 & 0.96 & -0.9 & 0.1  \\
    CCL5 & closed $w$CDM & 0.3 & 0.05 & 0.75 & 0.7 & 0.8 & 0.96 & -0.9 & 0.1  \\
    CCL6 & flat $\Lambda$CDM & 0.3 & 0 & 0.7 & 0.7 & 0.8 & 0.96 & -1 & 0 \\
    WMAP7 & flat $\Lambda$CDM & 0.272 & 0.0455 & 0.728 & 0.704 & 0.810 & 0.967 & -1 & 0 \\
    Planck 2013 & flat $\Lambda$CDM & 0.318 & 0.0490 & 0.682 & 0.671 & 0.834 & 0.962 & -1 & 0 \\
    \hline
  \end{tabular}
  \caption{Cosmological models with massless neutrinos used in testing \ccl against independently produced benchmarks.}
  \label{tab:cosmologies}
\end{table*}
